Article (Scientific journals)
Dusty plasma in active galactic nuclei
Czerny, Bożena; Zajaček, Michal; Naddaf Moghaddam, Mohammad Hassan et al.
2023In European Physical Journal D. Atoms, Molecules, Clusters and Optical Physics, 77 (4)
Peer Reviewed verified by ORBi
 

Files


Full Text
s10053-023-00630-8.pdf
Publisher postprint (1.25 MB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
Active galactic nuclei; Balmer lines; Dusty molecular torus; Dusty plasmas; Large viewing angle; Torus region; Atomic and Molecular Physics, and Optics
Abstract :
[en] Abstract: For many years we have known that dust in the form of a dusty-molecular torus is responsible for the obscuration in active galactic nuclei (AGN) at large viewing angles and, thus, for the widely used phenomenological classification of AGN. Recently, we gained new observational and theoretical insights into the geometry of the torus region and the role of dust in the dynamics of emerging outflows and failed winds. We will briefly touch on all these aspects and provide a more detailed update of our dust-based model (FRADO—Failed Radiatively Accelerated Dusty Outflow) capable of explaining the processes of formation of Balmer lines in AGN. Graphic abstract: [Figure not available: see fulltext.]
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Czerny, Bożena ;  Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland
Zajaček, Michal;  Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Brno, Czech Republic
Naddaf Moghaddam, Mohammad Hassan  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Space sciences, Technologies and Astrophysics Research (STAR) ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland ; Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland
Sniegowska, Marzena;  Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland ; School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel
Panda, Swayamtrupta;  Laboratório Nacional de Astrofísica, MCTI, Itajubá, Brazil
Różanska, Agata;  Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
Adhikari, Tek P.;  Inter University Center for Astronomy and Astrophysics, Pune, India
Pandey, Ashwani;  Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland
Jaiswal, Vikram Kumar;  Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland
Karas, Vladimír;  Astronomical Institute, Czech Academy of Sciences, Prague, Czech Republic
Borkar, Abhijeet;  Astronomical Institute, Czech Academy of Sciences, Prague, Czech Republic
Martínez-Aldama, Mary Loli;  Departamento de Astronomía, Universidad de Chile, Santiago, Chile
Prince, Raj;  Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland
More authors (3 more) Less
Language :
English
Title :
Dusty plasma in active galactic nuclei
Publication date :
April 2023
Journal title :
European Physical Journal D. Atoms, Molecules, Clusters and Optical Physics
ISSN :
1434-6060
eISSN :
1434-6079
Publisher :
Springer Science and Business Media Deutschland GmbH
Volume :
77
Issue :
4
Peer reviewed :
Peer Reviewed verified by ORBi
Funding text :
This project has received funding from the European Research Council (ERC) under the European Union\u2019s Horizon 2020 research and innovation program (Grant Agreement No. [951549]). The project was partially supported by the Polish Funding Agency National Science Centre, project 2017/26/A/ST9/00756 (MAESTRO 9), and MNiSW grant DIR/WK/2018/12. MLM-A acknowledges financial support from Millennium Nucleus NCN (TITANs). VK acknowledges the Czech Science Foundation Project No. 21-06825X \u201CAccreting black holes in the new era of X-ray polarimetry missions\u201D. SP acknowledges financial support from the Conselho Nacional de Desenvolvimento Cient\u00EDfico e Tecnol\u00F3gico (CNPq) Fellowship (164753/2020-6). MS acknowledges the financial support of the Polish Funding Agency National Science Centre 2021/41/N/ST9/02280 (PRELUDIUM 20). MZ acknowledges the financial support of the GA\u010CR EXPRO Grant No. 21-13491X \u201CExploring the Hot Universe and Understanding Cosmic Feedback\u201D. The authors also acknowledge the Czech-Polish mobility program (M\u0160MT 8J20PL037 and NAWA PPN/BCZ/2019/1/00069), the OPUS-LAP/GA\u010CR-LA bilateral project (UMO-2021/43/I/ST9/01352 and GF22-04053 L), and the Czech Ministry of Education, Youth and Sports Research Infrastructure (LM2023047).This project has received funding from the European Research Council (ERC) under the European Union\u2019s Horizon 2020 research and innovation program (Grant Agreement No. [951549]). The project was partially supported by the Polish Funding Agency National Science Centre, project 2017/26/A/ST9/00756 (MAESTRO 9), and MNiSW grant DIR/WK/2018/12. MLM-A acknowledges financial support from Millennium Nucleus NCN19 _ 058 (TITANs). VK acknowledges the Czech Science Foundation Project No. 21-06825X \u201CAccreting black holes in the new era of X-ray polarimetry missions\u201D. SP acknowledges financial support from the Conselho Nacional de Desenvolvimento Cient\u00EDfico e Tecnol\u00F3gico (CNPq) Fellowship (164753/2020-6). MS acknowledges the financial support of the Polish Funding Agency National Science Centre 2021/41/N/ST9/02280 (PRELUDIUM 20). MZ acknowledges the financial support of the GA\u010CR EXPRO Grant No. 21-13491X \u201CExploring the Hot Universe and Understanding Cosmic Feedback\u201D. The authors also acknowledge the Czech-Polish mobility program (M\u0160MT 8J20PL037 and NAWA PPN/BCZ/2019/1/00069), the OPUS-LAP/GA\u010CR-LA bilateral project (UMO-2021/43/I/ST9/01352 and GF22-04053\u00A0L), and the Czech Ministry of Education, Youth and Sports Research Infrastructure (LM2023047).
Available on ORBi :
since 12 January 2025

Statistics


Number of views
21 (2 by ULiège)
Number of downloads
9 (0 by ULiège)

Scopus citations®
 
12
Scopus citations®
without self-citations
8
OpenCitations
 
4
OpenAlex citations
 
11

Bibliography


Similar publications



Contact ORBi